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Physics

arXiv preprints from January 1, 2026 through July 20, 2026 — 03:40:02 EST

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Posted in cond-mat.mtrl-sci · 2026-01-16 · Jowon Onasanyab, Mourad Benamara, Kanagaraj Moorthi, H. O. H. Churchill, Bothina Hamad, M. O. Manasreh

Chemical Vapor Deposition Growth and Characterization of ReSe2

Two-dimensional (2D) flakes of ReSe2 structure were grown by chemical vapor deposition and investigated at room temperature using Raman, photoluminescence, and absorption spectroscopies. The Raman spectra revealed eighteen phonon modes in the range of 100-300 cm-1 that were found in good agreement with the density functional theory...

💬 0 commentsarXiv:2601.11726v1PDF
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Posted in cond-mat.mtrl-sci · 2026-01-16 · Timothy A. Elmslie, Luca Basso, Adam Dodson, Jacob Henshaw, Andrew M. Mounce

Homogeneous Microwave Delivery for Quantum Sensing with Nitrogen-Vacancy Centers at High Pressures

Nitrogen vacancy (NV) centers have been demonstrated as a useful tool in high pressure environments. However, the geometry and small working area of the diamond anvil cells (DACs) used to apply pressure present a challenge to effective delivery of microwave (mw) fields. We designed and characterized a novel slotted design for mw...

💬 0 commentsarXiv:2601.11725v1PDF
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Posted in physics.flu-dyn · 2026-01-16 · Sidian Chen, Bo Guo, Tianyuan Zheng

Coupled two-phase flow and surfactant/PFAS transport in porous media with angular pores: From pore-scale physics to Darcy-scale modeling

Two-phase surfactant-laden flow and transport in porous media are central to many natural and engineering applications. Surfactants alter two-phase flow by modifying interfacial tension and wettability, while two-phase flow controls surfactant transport pathways and interfacial adsorption. These coupled processes are commonly modeled...

💬 0 commentsarXiv:2601.11721v1PDF
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Posted in astro-ph.HE · 2026-01-16 · Andrea Gnarini, Swati Ravi, Philip Kaaret, Anna Bobrikova, Juri Poutanen, Sofia V. Forsblom, Francesco Ursini, Maria Cristina Baglio, Stefano Bianchi, Fiamma Capitanio, Massimo Cocchi, Maria Alejandra Diaz Teodori, Sergio Fabiani, Ruben Farinelli, Giorgio Matt, Mason Ng, Alexander Salganik, Paolo Soffitta, Antonella Tarana, Silvia Zane

Discovery of High X-Ray Polarization from the Neutron Star Low-Mass X-Ray Binary Cyg X-2 in the Horizontal Branch

We present results from simultaneous X-ray polarimetric and spectroscopic observations of the bright neutron star low-mass X-ray binary Cyg X-2, performed by the Imaging X-ray Polarimetry Explorer (IXPE) and the Nuclear Spectroscopic Telescope Array (NuSTAR). IXPE detected significant polarization (15 sigma) from the source in the 2-8...

💬 0 commentsarXiv:2601.11718v1PDF
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Posted in physics.ins-det · 2026-01-16 · Thorsten Buss, Henry Day-Hall, Frank Gaede, Gregor Kasieczka, Katja Krüger

AllShowers: One model for all calorimeter showers

Accurate and efficient detector simulation is essential for modern collider experiments. To reduce the high computational cost, various fast machine learning surrogate models have been proposed. Traditional surrogate models for calorimeter shower modeling train separate networks for each particle species, limiting scalability and...

💬 0 commentsarXiv:2601.11716v1PDF
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Posted in astro-ph.GA · 2026-01-16 · Nicolas Mazziotti, Michael G. Jones, Donghyeon J. Khim, David J. Sand, Paul Bennet

Blobs and Blurs: A Citizen Science-Identified Catalog of Diffuse Galaxies in the Fornax Cluster

We present a catalog of 643 diffuse galaxies identified through a citizen science search of the Fornax cluster, of which we estimate 21.8% are nucleated (139/637; 6 inconclusive). This marks the first crowd-sourced effort to construct a cluster-scale census of diffuse galaxies. These objects were visually identified using a...

💬 0 commentsarXiv:2601.11715v1PDF
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Posted in quant-ph · 2026-01-16 · Marco Riccardi, Aviv Glezer Moshe, Guido Menichetti, Riccardo Aiudi, Carlo Cosenza, Ashkan Abedi, Roberto Menta, Halima Giovanna Ahmad, Diego Nieri Orfatti, Francesco Cioni, Davide Massarotti, Francesco Tafuri, Vittorio Giovannetti, Marco Polini, Francesco Caravelli, Daniel Szombati

Experimental observation of dynamical blockade between transmon qubits via ZZ interaction engineering

We report the experimental realization of strong longitudinal (ZZ) coupling between two superconducting transmon qubits achieved solely through capacitive engineering. By systematically varying the qubit frequency detuning, we measure cross-Kerr inter-qubit interaction strengths ranging from 10 MHz up to 350 MHz, more than an order of...

💬 0 commentsarXiv:2601.11714v1PDF
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Posted in astro-ph.EP · 2026-01-16 · S. Mac Manamon, L. Matrà, S. Marino, A. Brennan, Y. Han, M. R. Jankovic, P. Weber, M. Bonduelle, J. M. Carpenter, G. Cataldi, A. M. Hughes, A. Kóspál, J. P. Marshall, B. C. Matthews, J. Milli, A. Moór, K. Öberg, S. Pérez, A. A. Sefilian, D. J. Wilner, M. C. Wyatt, E. Chiang, A. S. Hales, J. B. Lovell, P. Luppe, M. A. MacGregor, T. Pearce, M. Booth, C. del Burgo, A. Fehr, E. Mansell, B. Zawadzki

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) IV: CO gas imaging and overview

CO gas is detected in a significant number of debris discs, but its origin and evolution remains unclear. Key constraints are its mass and spectro-spatial distribution, which are coupled through optical depth and have only been analysed at low to moderate resolution so far. The ALMA survey to Resolve exoKuiper belt Substructures...

💬 0 commentsarXiv:2601.11712v1PDF
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Posted in astro-ph.EP · 2026-01-16 · S. Marino, V. Gupta, P. Weber, T. D. Pearce, A. Brennan, S. Pérez, S. Mac Manamon, L. Matrà, J. Milli, M. Booth, C. del Burgo, G. Cataldi, E. Chiang, Y. Han, Th. Henning, A. M. Hughes, M. R. Jankovic, Á. Kóspál, J. B. Lovell, P. Luppe, E. Mansell, M. A. MacGregor, A. Moór, J. Olofsson, A. A. Sefilian, D. J. Wilner, M. C. Wyatt, B. Zawadzki

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) VIII: A dust arc and non-Keplerian gas kinematics in HD 121617

ExoKuiper belts around young A-type stars often host CO gas, whose origin is still unclear. The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) includes 6 of these gas-bearing belts, to characterise their dust and gas distributions and investigate the gas origin. As part of ARKS, we observed the gas-rich system HD121617 and...

💬 0 commentsarXiv:2601.11711v1PDF
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Posted in astro-ph.GA · 2026-01-16 · B. T. Draine

Resonant Scattering of the He I 1.0833$μ$m Triplet in H II Regions: Emission Spectra

Resonant scattering of He I 1.0833$μ$m triplet photons by metastable He 2 $^3$S$_1$ is studied for optical depths characteristic of H II regions. Regions with large He 2 $^3$S$_1$ column densities are predicted to have unusually broad, multi-peaked 1.0833$μ$m emission profiles, with the centroid blue-shifted by up to $\sim$14 km/s...

💬 0 commentsarXiv:2601.11710v2PDF
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Posted in astro-ph.SR · 2026-01-16 · Conaire Deagan, Benjamin T. Montet

Inferring hemispheric asymmetries of stellar active regions through the information content of astrometric signals

Photometric light curves suffer from fundamental degeneracies that limit surface information recovery. We demonstrate that astrometry enables access to complementary information through photocentre variations induced by rotating surface features. The forthcoming commissioning of microarcsecond-precision astrometric missions presents...

💬 0 commentsarXiv:2601.11707v2PDF
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Posted in astro-ph.EP · 2026-01-16 · S. Marino, L. Matrà, A. M. Hughes, J. Ehrhardt, G. M. Kennedy, C. del Burgo, A. Brennan, Y. Han, M. R. Jankovic, J. B. Lovell, S. Mac Manamon, J. Milli, P. Weber, B. Zawadzki, R. Bendahan-West, A. Fehr, E. Mansell, J. Olofsson, T. D. Pearce, A. Bayo, B. C. Matthews, T. Löhne, M. C. Wyatt, P. Ábrahám, M. Bonduelle, M. Booth, G. Cataldi, J. M. Carpenter, E. Chiang, S. Ertel, A. S. Hales, Th. Henning, Á. Kóspál, A. V. Krivov, P. Luppe, M. A. MacGregor, J. P. Marshall, A. Moór, S. Pérez, A. A. Sefilian, A. G. Sepulveda, D. J. Wilner

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) I: Motivation, sample, data reduction, and results overview

The outer regions of planetary systems host dusty debris discs analogous to the Kuiper belt (exoKuiper belts), which provide crucial constraints on planet formation and evolution processes. ALMA dust observations have revealed a great diversity, and that some belts contain CO gas, whose origin and implications are uncertain. Most of...

💬 0 commentsarXiv:2601.11708v1PDF
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Posted in gr-qc · 2026-01-16 · Marina De Amicis, Enrico Cannizzaro

Post-Minkowskian expansion of the Prompt Response in a Schwarzschild background

We study the early-time component of the Green's function of a Schwarzschild black hole, traveling on the curved light cone and usually denoted as the prompt response. Working in a post-Minkowskian approximation, we show for the first time that the prompt response is given by the residue of poles at $ω=0$ present in the complex...

💬 0 commentsarXiv:2601.11706v1PDF
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Posted in astro-ph.EP · 2026-01-16 · Philipp Weber, Sebastián Pérez, Clément Baruteau, Sebastian Marino, Fernando Castillo, Marija R. Jankovic, Tim Pearce, Mark C. Wyatt, Antranik A. Sefilian, Johan Olofsson, Gianni Cataldi, Joshua B. Lovell, Carlos del Burgo, A. Meredith Hughes, Sorcha Mac Manamon, Aoife Brennan, Luca Matrà, Julien Milli, Brianna Zawadzki, Eugene Chiang, Meredith MacGregor, David J. Wilner, Myriam Bonduelle, John Carpenter, Yinuo Han, Ágnes Kóspál, Patricia Luppe

The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) IX: Gas-driven origin for the continuum arc in the debris disc of HD 121617

Debris discs were long considered to be largely gas-free environments governed by collisional fragmentation, gravitational stirring, and radiative forces. Recent CO detections show that gas is present, but its abundance and origin remain uncertain. The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) revealed a narrow gas...

💬 0 commentsarXiv:2601.11709v1PDF
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Posted in astro-ph.GA · 2026-01-16 · J. M. Diego, J. M. Palencia, C. Goolsby, C. J. Conselice, D. J. Lagattuta, G. Mahler, J. Richard, K. Sharon, L. L. R. Williams

Hedorah, the first yellow supergiant Kaiju star candidate at $z\approx3$ revealed by behind AS1063

We present a new free-form lens model for the $z=0.348$ galaxy cluster AS1063, based on previously spectroscopically confirmed lensed galaxies and new images from the GLIMPSE program. We use the ultra-deep data to identify new counterimages for previously confirmed (spectroscopically) lensed systems. We use the full set of...

💬 0 commentsarXiv:2601.11704v1PDF
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Posted in hep-ph · 2026-01-16 · Marco Chianese, Ninetta Saviano, Sara Cesare, Vincenzo M. Grieco, Valentina Nasti, Francesca Spinnato, Alessandro Tiano

Probing super-heavy dark matter with ultra-high-energy gamma rays

We refine the constraints on the lifetime of decaying super-heavy dark matter particles (SHDM), with masses ranging from $10^7$ to $10^{15}$ GeV, by analyzing ultra-high-energy (UHE) gamma-ray data. Our approach involves an accurate comparison of the primary gamma-ray emissions resulting from prompt SHDM decays in the galactic halo...

💬 0 commentsarXiv:2601.11703v1PDF
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Posted in hep-th · 2026-01-16 · Henriette Elvang, Aidan Herderschee, Roger Morales

String Theory from Maximal Supersymmetry

We explore the space of non-gravitational, maximally supersymmetric, planar 4d effective field theories (EFTs) that have $\mathcal{N}=4$ super Yang-Mills (SYM) at leading order. We show that in the weakly-coupled regime, highly non-trivial nonlinear constraints on the 4-point Wilson coefficients follow from enforcing $\mathcal{N}=4$...

💬 0 commentsarXiv:2601.11705v2PDF
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Posted in astro-ph.HE · 2026-01-16 · Andrew G. Sullivan, Jack T. Dinsmore, Roger W. Romani

X-ray Polarization of the Intrabinary Shock in Redback Pulsar J1723$-$2837

The intrabinary shocks (IBS) in spider pulsars emit non-thermal synchrotron X-rays from accelerated electrons and positrons in the shocked pulsar wind, likely energized by magnetic reconnection. The double-peaked X-ray light curves from these shocks have been well characterized in several spider systems. In this paper, we analyze...

💬 0 commentsarXiv:2601.11521v1PDF
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Posted in cond-mat.supr-con · 2026-01-16 · Sebastian Allende, David Galvez-Poblete

Vacuum-selected timescales in driven Josephson systems

In this work, we demonstrate that the intrinsic timescale of a Josephson junction can be controlled through dynamical vacuum selection. By applying a Kapitza-like high-frequency drive to the system, the effective Josephson potential is reshaped, allowing for the stabilization of inphase or antiphase configuration. As a result, the...

💬 0 commentsarXiv:2601.11519v1PDF
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Posted in physics.soc-ph · 2026-01-16 · Tzula B. Propp, Brandy Todd, Sara A. Metwalli, Alina Helena S. Gallardo, Michael Dascal, Denise Ruffner, Klaus D. Jöns, Shaeema Zaman, Judith Kreukels, Marilù Chiofalo, Lydia Sanmartí-Vila

Meeting the Needs of the Global Quantum Science Community: A Call to Action

2025 marks one hundred years since the discovery of quantum mechanics. In the century since then, quantum science has blossomed into a global community composed of academics, engineers, developers, and entrepreneurs. The world is currently in the middle of the so-called second quantum revolution, with increased public awareness of...

💬 0 commentsarXiv:2601.14297v3PDF
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Posted in astro-ph.GA · 2026-01-16 · Callum T. Donnan, Derek J. McLeod, Ross J. McLure, James S. Dunlop, Fergus Cullen, Mark Dickinson, Pablo Arrabal Haro, Anthony J. Taylor, Cecilia Bondestam, Feng-Yuan Liu, Karla Z. Arellano-Córdova, Laia Barrufet, Ryan Begley, Adam C. Carnall, Hanna Golawska, Ho-Hin Leung, Dirk Scholte, Thomas M. Stanton

Spectroscopic confirmation of a large and luminous galaxy with weak emission lines at $\mathbf{z = 13.53}$

We present JWST/NIRSpec PRISM observations of a robust galaxy candidate at $z\simeq14$, selected from pure-parallel NIRCam imaging; PAN-z14-1. The NIRSpec spectrum allows confirmation of this source at $z_{\rm spec}=13.53^{+0.05}_{-0.06}$ through modeling of the Lyman-$α$ break. PAN-z14-1 is the fourth most distant galaxy known to...

💬 0 commentsarXiv:2601.11515v2PDF
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Posted in cond-mat.mtrl-sci · 2026-01-16 · Brian Lee, Linna Qiao, Samuel Gleason, Guangwen Zhou, Xiaohui Qu, Judith Yang, Jim Ciston, Deyu Lu

Predictive autoencoder-transformer model of Cu oxidation state from EELS and XAS spectra

X-ray absorption spectroscopy (XAS) and electron energy-loss spectroscopy (EELS) produce detailed information about oxidation state, bonding, and coordination, making them essential for quantitative studies of redox and structure in functional materials. However, high-throughput quantitative analysis of these spectra, especially for...

💬 0 commentsarXiv:2601.11509v1PDF
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Posted in cond-mat.other · 2026-01-16 · Robert J. Vukelich, Tenzin Norden, Tracy G. Hastings, Mohan Giri, Michelle Caldwell, Shabnam Forutan, John L. Reno, David J. Hilton

Broadband Terahertz Time-domain Spectroscopy of Quantum Materials in a Dilution Refrigerator

We have constructed a terahertz time domain spectroscopy system using a Bluefors dilution refrigerator with a 7 T split-coil magnet. Using a gallium arsenide single quantum well sample, terahertz waveforms were measured at 145 mK in a magnetic field range from 0 to 6 Tesla to measure cyclotron resonance. Effective mass is found to be...

💬 0 commentsarXiv:2601.11506v1PDF
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Posted in cond-mat.str-el · 2026-01-16 · Sandy Adhitia Ekahana, Aalok Tiwari, Souvik Sasmal, Zefeng Cai, Ravi Kumar Bandapelli, I-Hsuan Kao, Jian Tang, Chenbo Min, Tiema Qian, Kenji Watanabe, Takashi Taniguchi, Ni Ni, Qiong Ma, Chris Jozwiak, Eli Rotenberg, Aaron Bostwick, Simranjeet Singh, Noa Marom, Jyoti Katoch

Visualization of Tunable Electronic Structure of Monolayer TaIrTe$_4$

Monolayer TaIrTe$_4$ has emerged as an attractive material platform to study intriguing phenomena related to topology and strong electron correlations. Recently, strong interactions have been demonstrated to induce strain and dielectric screening tunable topological phases such as quantum spin Hall insulator (QSHI), trivial insulator,...

💬 0 commentsarXiv:2601.11504v1PDF